Chronology of a probable neotectonic Pleistocene rock avalanche
Transcription
Chronology of a probable neotectonic Pleistocene rock avalanche
ARTICLE IN PRESS Quaternary International 148 (2006) 138–148 Chronology of a probable neotectonic Pleistocene rock avalanche, Cordon del Plata (Central Andes), Mendoza, Argentina Stella M. Moreiras Instituto Argentino de Nivologı´a, Glaciologı´a y Ciencias Ambientales (IANIGLA) – CRICYT, CONICET, Av. Dr. Ruiz Leal s/n, Parque, (5500) Mendoza, Argentina Casilla Correo 330 Available online 19 January 2006 Abstract Placetas Amarillas-1 rock avalanche located at 321430 S–691250 W was geomorphologically, stratigraphically and chronologically studied. This extraordinary event dammed a secondary gully causing the formation of a barrier-lake, indicated by relict lacustrine and diatomite deposits. Stratigraphically, its deposit is overlain by alluvial fans where three tephra layers are intercalated. Dating using Ar–Ar method of the middle ash level at 350780 ka determined a Middle Pleistocene or older age for this event. Furthermore, the younger age of Placetas Amarillas-2 is established by relative dating techniques such as soil development and rock varnish development. The ages established in this research indicate that Placetas Amarillas-1 may be temporally correlated with the Tigre Dormido rock avalanche, suggesting that the occurrence of these rock avalanches may be related to regional neotectonic activity. Nevertheless, climatic conditions are not underestimated as the Tigre Dormido event occurred before formation of an outwash terrace related to a glaciation of Early Middle Pleistocene age. r 2005 Elsevier Ltd and INQUA. All rights reserved. 1. Introduction Rock avalanches, known also as sturzstroms, are large, extremely rapid and often open-slope flows (Cruden and Varnes, 1996). Relatively large volumes and extremely high velocities associated with this kind of flow activity are often linked to a catastrophic impact. Historical examples included the Goldau slide of 1806 (volume 30–40 Mm3, estimated velocity 70 m/s, 457 deaths); the Elm slide of 1881 (volume 11 Mm3, estimated velocity 70 m/s, 115 deaths); and the Frank slide of 1903 (volume 30 Mm3, estimated velocity 28 m/s, 70 deaths) (Heim, 1919, 1932; Abele, 1974; Cruden and Krahn, 1978; Hsü, 1978; Cruden and Hungr, 1986). The research community has a particular interest in the survey of these huge landslides, concerning probable causes, rupture mechanisms, velocities, magnitudes, volumes and probable relations with certain climatic conditions (Panizza, 1973; Abele, 1974; Hsü, 1975; Plafker and Ericksen, 1978; Voight and Corresponding author. Tel.: +54 0261 4287029; fax: +54 0261 4285940. E-mail address: [email protected]. Pariseau, 1978; Adams, 1981; Záruba and Mencl, 1982; Keefer, 1984; Gonzalez Diez et al., 1996; Poschinger and Haas, 1997; Trauth and Strecker, 1999; Corsini et al., 2000; Hermanns et al., 2000, 2001; Trauth et al., 2000; Borgatti et al., 2001; Corsini et al., 2001). As the study area is a seismic region, several landslides have been triggered by earthquakes with magnitudes higher than 3.5, and others are frequently related to intense rainstorms (Moreiras, 2003a, 2004a, 2005a,b). Even though debris flows and rockfalls are more common events, huge rock avalanches have affected the region (Salomón, 1979; Espizúa and Bengochea, 1991; Fauqué et al., 2000, 2001; Moreiras, 2003b, 2004b). These extraordinary events have usually dammed valleys and represent a potential hazard for this developing mountain area, where intense tourist activity exists. As well, the International road to Chile, an important traffic route, and the older International Transandino Railway pass through the area. Although, these huge landslides have been geomorphologically studied, numerical dating of their deposits and assessment of their probable causes are still lacking. Establishing the chronology of these exceptional landslides is essential to understand their causes and relationship with 1040-6182/$ - see front matter r 2005 Elsevier Ltd and INQUA. All rights reserved. doi:10.1016/j.quaint.2005.11.009 ARTICLE IN PRESS S.M. Moreiras / Quaternary International 148 (2006) 138–148 past climatic conditions. Brundsen (1979) remarked that different hypothesis on the nature of rock avalanche movement mechanism have been proposed, unfortunately without complete satisfactory explanation; and lacking on precise triggering causes do not allow or enable realistic prediction of these threatening events. Present study enhances the knowledge of two extraordinary events identified in the study area. Chronology established for one of them, Placetas Amarillas-1 rock avalanche, allow temporal correlation with other rock avalanche studied previously, suggesting they may be sourced by the same triggering factor and at the same conditions. Probable triggering factor is analyzed regarding potential hazard evaluation. 2. Location of the study area The study area is located in north-western Mendoza province at 321430 S latitude and 691250 W longitude. It comprises a 33 km2 area along Placetas Amarillas. It is 139 situated near La Quinta place, directly south of the Uspallata railway station (Fig. 1), access to the area is via International highway N1 7 to Chile, and then following unconsolidated road along La Quinta gully from the old Uspallata railway station. Tourist facilities and a small artificial dam have been built in La Quinta. 3. Geological/geographical setting The study area comprises the Cordillera Frontal geological province, characterized with strong relief and very steep slopes. The highest elevations are: Colorado (4790 m.a.s.l.), Division (4603 m.a.s.l.), Burro (4293 m.a.s.l.), and Minero (3813 m.a.s.l.) peaks. A Permo-Triassic volcanic complex (Choiyoi Group) crops out in the region, composed of pyroclastic material, lavas, subvolcanic and intrusive rocks. The Tambillos and Horcajo Formations can be distinguished. The former is mainly constituted by volcanites, rhyolitic lavas and lacustrine sediments (Cortés, 1985). The latter corresponds Fig. 1. Location of study area, where six huge landslides are identified: (a) Tigre Dormido (TD); (b) Placetas Amarillas 1 (PA-1); (c) Placetas Amarillas 2 (PA-2), c-Piedras Blancas 1 (PB-1); (d) Piedras Blancas 2 (PB-2); (e) Piedras Blancas 3 (PB-3), and (f) Burro (BU) (after Fauqué et al., 2000, 2001). Pleistocene drifts identified in the area are the Uspallata terminal moraine (UM), Uspallata outwash (UO), and Punta de Vacas outwash (PO) (after Espizúa, 1993; Moreiras, 2003, 2004b). Placetas Amarillas fault (PA) and Piedras Blancas fault (PB) are represented. ARTICLE IN PRESS 140 S.M. Moreiras / Quaternary International 148 (2006) 138–148 to rhyolitic—dacitic pyroclastic rocks and lavas (Mirré, 1966). The Choiyoi Group subvolcanic rocks are represented by rhyolitic porphyries and andesitic dikes. A larger porphyry body outcrops in the Colorado and Minero peaks, dated to 278710 Ma (Caminos et al., 1979) by K/Ar (Early Permian). Intrusive rocks are constituted by small granitic and gabbroic bodies dated at 244710 Ma by K/Ar (Caminos et al., 1979). Quaternary sediments are formed by alluvial and colluvial deposits. Moreover, in this sector, two outwash terraces can be identified along the Mendoza river; one is related to the Punta de Vacas Glaciation, correlated with isotopic oxygen stage 6 (Espizúa and Bigazzi, 1998) and the other outwash terrace is related to the Uspallata Glaciation, considered as at least Early Middle Pleistocene (Espizúa, 1993). A terminal moraine belonging to the Uspallata Glaciation was identified in the Uspallata valley (Espizúa, 1993) (Fig. 1). Several landslide deposits have been also identified along the Mendoza river valley (Moreiras, 2003a, 2004a,b, 2005a). 4. Tectonic framework Convergence of Nazca and Sudamericana plates, located 300 km westward, generated a compressive regimen that has been maintained until present. At the latitude of the survey area, a flat segment of the Nazca Plate approximately 100 km deep has been linked to an intense intraplate seismic activity and notable neotectonic activity (Bastı́as et al., 1993; Ramos, 1993). Although historical material prior to the conquest period and the following three centuries is scarce, earthquakes with magnitudes greater than seven have been reported in the region during the last two centuries (INPRES, 1993) (Fig. 2). This sector of the Central Argentine Andes is characterized by active tectonic uplift (Ramos, 1993). Structurally, the study area is characterized by thrust tectonics along the eastern margin of the Cordillera Frontal, evidenced by reverse faults of the Carrera fault system called the Espolón de la Carrera by Polanski (1958). According to Kozlowski et al. (1993), this fault system is responsible for the uplift of the Cordillera Frontal during Pliocene–Lower Pleistocene. The Placetas Amarillas and Piedras Blancas faults, related to this system, affect the region with eastern vergence. The former has a northern–southern trend dipping 57–731W and putting in contact intrusive and volcanite rocks with Tertiary sediments. The Piedras Blancas fault has a north–south trend at the southern end, and trends northwest–southeast near Tabolango pampa dipping 54–571W (Cortés, 1993). 5. Methodology In the Placetas Amarillas area, at least two landslide deposits were initially identified by photointerpretation of air photos (1: 50,000 scale) and satellite images (Fauqué et al., 2000, 2001). They were classified as rock avalanches. However, in this study this classification for one of them is re-assessed based on the Multilingual Landslide Glossary (WP/WLI, 1993), Hutchinson (1988) and Angeli et al. (1996). The events were studied in detail from a stratigraphic point of view. Identification and Ar–Ar dating of an ash level intercalated in alluvial fans that overlies the deposit of PA-1 rock avalanche allowed determination of the maximum age for this event. Relative-age criteria such as soil development and rock varnish development were used to establish the tentative chronology of landslide events in the Placetas Amarillas (Blackwelder, 1931; Sharp and Birman, 1963; Sharp, 1969, 1972; Birkeland, 1973; Burke and Birkeland, 1979; Colman and Pierce, 1986; Ritter, 1987; Wells et al., 1987a,b; Knuepfer, 1988). Soil profiles were analyzed in natural cuts and were classified according to procedures and terminology suggested by Birkeland (1984). Horizon size distribution was determined using 0.34 mm and 0.20 mm sieves, and retained fractions were weighed using a electronic balance (Metter PN 1210) with 10 mg accuracy. The fraction smaller than 0.2 mm was analyzed by the dispersion method. Carbonate content was determined by a volumetric method, and a Orion pehachimeter with 5, 7 and 8 patrons was used for pH determination. Effervescence grade was established with hydrochloric acid (1 N). Rock varnish development was observed on boulders larger than 10 cm randomly selected within an area of 10 10 m. Boulders were classified as: unvarnished: varnished surface less than 10%; slightly varnished: varnished surface more than 10% and less than 50%; moderately varnished: varnished surface between 50–90%; and varnished: more than 90% of boulder surface varnished. 6. Previous work In the study area, huge volumes of debris material were mobilized in proximal areas. Fauqué et al. (2000) identified six rock avalanches: (a) Tigre Dormido (TD), (b) Placetas Amarillas 1 (PA-1), (c) Placetas Amarillas 2 (PA-2), (d) Piedras Blancas 1 (PB-1), (e) Piedras Blancas 2 (PB-2), and (f) Piedras Blancas 3 (PB-3) (Fig. 1). Initially, these deposits were mapped as tectonic breccias during research on Geological Sheet 3369-15 Potrerillos (Cortés, 1993; Folguera et al., 2000). Fauqué et al. (2000, 2001) proposed that the triggering factor of these rock avalanches was a seismic movement associated with neotectonic activity of Placetas Amarillas and Piedras Blancas faults. As well, these authors suggested that rock avalanches occurred during Upper Middle Pleistocene–Holocene. They observed an ash level underlying rock avalanche deposits and tentatively correlated it with an ash level dated 360736 ka by Espizúa (1993). Pleistocene glaciations occurred along Rio Mendoza valley, have been studied by Espizúa (1993) from Aconcagua peak to Uspallata valley. This author recognized two outwash terraces related to the Punta de Vacas and Uspallata Pleistocene glaciations in Uspallata valley. Later, ARTICLE IN PRESS S.M. Moreiras / Quaternary International 148 (2006) 138–148 141 Fig. 2. (a) Seismic zone linked to flat subduction segment of Nazca plate; and (b) Earthquakes from XX century and some from XVI century (after Moreiras, 2004a,b). Moreiras (2003b, 2004b) identified different outwash remnants eastern of the Uspallata valley. As these deposits are stratigraphically related to the Tigre Dormido rock avalanche, this author applied relative-age criteria with the aim to correlate these outwash deposits with those previously identified by Espizúa (1993). Based on varnish development, weathering degree measured on surfaces of dacite blocks, and topographic relations; these outwash deposits could be correlated with Uspallata and Punta de Vacas drifts (Moreiras, 2003b). Uspallata outwash remnants surround the deposit of Tigre Dormido rock avalanche in the neighboring La soltera gully. Moreover, remnants of lacustrine sediments belonging to this rock avalanche dammed lake are also surrounded by this outwash up stream of Soltera gully. For this reason, Moreiras (2004b) suggested that the Tigre Dormido rock avalanche is older than this outwash. As the Uspallata glaciation was assigned to at least Early Middle Pleistocene age (Espizúa and Bigazzi, 1998), the Tigre Dormido rock avalanche must have happened before or during this time period. 7. Placetas Amarillas events In Placetas Amarillas, Placetas Amarilllas-1 (PA-1) and Placetas Amarillas-2 (PA-2) landslides were identified (Fig. 3). In the former, originated on the eastern hillslope of the Minero peak (3813 m.a.s.l.), material moved to the opposite side of the Placetas Amarillas gully, and then, moved northward. Detrital material flowed down slope through the La Quinta and Libélulas gullies 7 km from the source area, reaching the proximity of the Uspallata ARTICLE IN PRESS 142 S.M. Moreiras / Quaternary International 148 (2006) 138–148 Fig. 3. (a) Drawing showing Placetas Amarillas landslides where two deposits of PA-1 are observed (a and b), location of lacustrine sediments at sites 1 and 2 is given; and (b) Panoramic view of PA-1 and PA-2 (after Fauqué et al., 2000, 2001; Moreiras, 2004b). railway station. The material traveled 2000 m topographically downslope, and was preserved along gullies, locally covering Choiyoi Group outcrops. The PA-2 event originated in the Placetas Amarillas headwaters. In this mass-movement, chaotic material moved approximately 1500 m horizontally and 170 m vertically (H/L0.11). A rock avalanche is a large bulk of mostly dry rock debris derived from the collapse of a slope or cliff, moving at a high velocity and for a long distance, even on a gentle slope. These complex events can be developed in two ways: by slide or fall of rock body continuing as a debris avalanche; or by sudden mobilization of a debris deposit by means of debris avalanche and debris flow (Angeli et al., 1996). Generally, rock avalanche deposits are tongue-like, lobate, with marked aerial delimitation, large volume, and great extent. PA-1 is a rock avalanche, as was initially classified by Fauqué et al. (2000). Mechanism analysis indicate two stages: an initial rupture and following material streaming, with associated morphological features. Furthermore, it seems to have been an extremely rapid movement of high velocity traveling a large distance. PA-2 does not have some characteristics of a primary rock avalanche. Although this event was sourced in a steep slope (351) it does not appear to have had a high velocity run-out of rock debris. As well, it is not a complex event, and thus PA-2 should be classified as a slide with a discrete displacement. Hutchinson (1988) pointed out that there is a transition from rockslides of moderate displacement that remains as blocks on the surface of rupture to slides on steeper and longer surfaces that break up into debris or transform into strurstroms. 8. Deposit characteristics The PA-1 rock avalanche has been preserved in two deposits: a rounded-hill with 400 m elevation eroded in the Fig. 4. Angular and sub-angular blocks and gravels, with diameter between 0.07 and 3 m, randomly distributed. central part; and a relict deposit with a different elongated morphological pattern. This deposit displays an undulating gentle surface morphology; with hollows containing small surface ponds. Its elongate form is exposed along the La Quinta and Las Libélulas gullies. Both deposits may correspond to two separate episodes (Fig. 3) (Fauqué et al., 2001). They cover an area of 7 km2 approximately with an estimated volume of 1 109 m3. The PA-1 chaotic deposit is poorly sorted, constituted by blocks of different sizes embedded in a finer matrix where the sand fraction predominates. Angular and sub-angular blocks and gravel with diameters between 0.07 and 3 m are randomly distributed (Fig. 4). The assemblage is of heterogeneous composition, with volcanic, sandstone, and rhyolitic blocks dominating that correspond to lithologies outcropping in the source area. Rock avalanches are characterized by uniform texture, unsorted material, monolithologic block composition that is conditioned by ithologies outcropping in the source area, and angular– subangular blocks (Hewitt, 1999). ARTICLE IN PRESS S.M. Moreiras / Quaternary International 148 (2006) 138–148 Fig. 5. Laminated or banded aspect of the deposit. Different color layers are associated with hydrothermal alteration. The PA-1 deposit is matrix-supported; the matrix proportion is more than 40%, although block-supported structure is observed in some sectors. The deposit shows diverse tones as a consequence of hydrothermal alteration of the original material. Silicification and manganese concentrations also exist. Different color-layers due to hydrothermal alteration attribute laminated or banded aspect (Fig. 5). Similar hydrothermal alteration was observed in the Tigre Dormido rock avalanche (Moreiras, 2003b). PA-2 corresponds to a lobate deposit with a high slope in the frontal part (351). It has an extent area of 3 km2 and its estimated volume is 2.5 108 m3. The deposit is matrixsupported with blocks of different sizes from a few centimeters to meters in diameter. Blocks are rhyolites with strong hydrothermal alteration: intense silication and chlorite minerals were observed. The largest blocks are composed by a breccia cemented by manganese, quartz and amorphous silica. 9. Source area features Outcrops in the source area, composed of rhyolite porphyry and volcanite rocks, are intensively jointed. Breccia zones related to these intense fractured rocks are observed. Cortés et al. (1999) have also mentioned the existence of breccias related to Piedras Blancas fault. Space between joints is variable from millimeters to meters, and orientations also are variable, with predominating northern–southern and northwest–southeast trends. These outcrops are also affected by intense hydrothermal alteration, indicated by intense silicification. Silica veins, stockwork structures and manganese concentration are observed. Moreover, feldspar grains in porphyries are completely replaced by clays. Copper oxides have been also identified such as azurite and malachite. Several breccia boulders and clasts cemented by silica or manganese oxides have been found. 143 PA-1 and PA-2 source areas are also characterized by steep slopes and relief contrast. The main scarps dip 551E and 401N, respectively. These lithological and topographical conditions probably favored and controlled slope instability in this region. The other rock avalanches identified, such as TD, PB-1, PB-2 and PB-3, also originated in areas with similar characteristics: topographical relief, lithologies affected by hydrothermal alteration, and intense jointing probably related to regional faults. As a consequence, structures, lithologies, and topographic contrast seem to be key conditioning factors for rock avalanche occurrence in this sector of Cordon del Plata. In Voight and Pariseau (1978)0 s opinion, several parameters such as lithology, structure, previous slope movements and climate favor rock avalanche occurrence. 10. Evidence of paleo-lake The extraordinary PA-1 event dammed the Minero gully causing the formation of a barrier-lake (Fauqué et al., 2001). A sequence of lacustrine sediments 38 m thick has been identified at site 1 (see Fig. 3) composed by intercalated sand and silt layers. Lower sediments are rich in organic matter, while in the upper 4 m, at 2238 m.a.s.l., fine sands predominate. Relict diatomite levels deposits were also observed in Minero gully margins (site 2) at 2120 m.a.s.l., approximately 60 m above the present gully bed, and thus the paleo-lake was not very deep (Fig. 6). The diatomite deposits are carbonate rich, showing violent effervescence with HCI (1 N), and have a high content of volcanic glass probably due to volcanic eruptions during the lake’s existence. Samples of lacustrine sediments were microscopically analyzed, and the diatom species determined were: Amphora sp., Achnates longipes, Central, Cymbella af. cistula cymbiformis, Cymbella ventricosa, Denticula, Fragilaria brevistriata var. Trigona, Gomphonema sp., Navicula sp., Neidium sp., and Nitzchia sp. Unfortunately these species are cosmopolite, and for this Fig. 6. Sequence of lacustrine sediments at site 1, where it can be also observed diatomite deposits at 2200 m.a.s.l. in the Minero gully (site 2). ARTICLE IN PRESS 144 S.M. Moreiras / Quaternary International 148 (2006) 138–148 reason, it was not possible to determine the paleo-climatic environment of the lake. Furthermore, the paleo-lake extent could not be established due to the limited outcrops of lacustrine deposit. These deposits were probably eroded along the Minero gully as a result of the collapse of the dam forced by the Piedras Blancas-3 rock avalanche (PB-3). 11. Chronology Along La Quinta and Las Libélulas gullies, the PA-1 rock avalanche deposit is overlain by alluvial fans where three ash levels are intercalated (Fig. 7). This volcanic material probably comes from active volcanic centers located southward of the study area such as Tupungatito (5913 m.a.s.l.), San José (6111 m.a.s.l.), and Maipo (5323 m.a.s.l.) stratovolcanoes. Numerical dating of medium ash level by Ar40–Ar39 gave an age of 350780 ka. Sampling of the lower ash level was not possible due to the irregular topography. The date suggests that, as the PA-1 rock avalanche is older than this ash level, the maximum age for the PA-1 rock avalanche should be Middle Pleistocene. However, the PA-2 chronology could not be inferred using stratigraphic relationships. 12. Relative dating techniques In order to establish a chronological sequence for the Placetas Amarillas landslides (PA-1 and PA-2), relative dating techniques, including soil and rock varnish development, were used. These techniques are time dependent, so they are frequently used for dating deposits (Blackwelder, 1931; Sharp and Birman, 1963; Sharp, 1969, 1972; Birkeland, 1973; Burke and Birkeland, 1979; Colman and Pierce, 1986; Knuepfer 1988; Wells et al., 1987a,b, Ritter, 1987). Fig. 7. Ash level intercalated in alluvial fans, dated 350780 ka by Ar–Ar method, overlying the PA-1 rock avalanche deposit. Filled arrow indicates contact between alluvial fans and PA-1 rock avalanche deposit. The PA-1 deposit shows discontinuous particles of sandy soils with A/B/C profile. The At horizon containing significant organic accumulation, although horizons generally erode. The horizon B reaches 20 cm thickness. It has a moderate laminate structure, 5 YR 5/2 color, and violently effervescence with HC1 (1 N). The horizon was classified as a Bk, and carbonate content reaches 7.5 mg/kg. Grain size distribution indicates that there is no clay enrichment in comparison to horizon C. Geochemical analysis for this horizon indicate 2.39% organic matter. In the PA-2 surface, a similar soil profile is observed, but the development of horizon AL is very variable, never thicker than 5 cm. Horizon B is 40 cm thicker, 5 YR 7/2, and has a pH of 7.65. In this horizon, 5 mg/kg carbonates and 0.76% of organic matter were determined, both parameters being lower than those determined in horizon BK of the PA-1 deposit. Previous studies in the region mentioned that carbonate content is the best indicator of soil development (Espizúa, 1993; Moreiras, 2004b). Rock varnish development on rhyolite blocks is greater in the PA-1 deposit than in the PA-2 deposit (Table 1), and differences also exist between two deposits of PA-1 (a and b). Sample areas were restricted due to intense disintegration on the larger blocks situated on the deposit surface, which may mask relative dating results as has been pointed out in previous works (Moreiras, 2003b, 2004b). 13. Discussion The PA-1 rock avalanche occurred before 350780 ka consistent with the age obtained in this study for the tephra layer overlying this deposit (see Fig. 7). As well, the TD rock avalanche occurred prior to the formation of the outwash terrace related to the Uspallata Glaciation, assigned to the Early Middle Pleistocene according to stratigraphic evidence (Moreiras, 2004b). Initially, Cortés (1993) tentatively proposed that the Placetas Amarillas Formation, corresponding to the six rock avalanche deposits identified in the region, should be older than the Uspallata Glaciation. The proximity of the rock avalanche source areas (approximately 4 km) may suggest their temporal correlation. The PA-1 and TD rock avalanches could originate from the same triggering factor and under the same conditions. Seismic shaking was probably the triggering factor of these rock avalanches in accordance with seismic history of this region (see Fig. 2). Keefer (1984) noted that these kinds of events are commonly caused by high magnitude earthquakes in seismic regions around the world. As earthquakes are generally associated with region of active faulting in continental interior, huge landslides have occurred in active tectonically regions (Plafker and Ericksen, 1978; Adams, 1981; Keefer, 1984; Perucca and Moreiras, 2003a,b). Furthermore, Hermanns and Strecker (1999) and Hermanns et al. (2000) mentioned landslide clusters along neotectonically active mountain fronts. Rock ARTICLE IN PRESS S.M. Moreiras / Quaternary International 148 (2006) 138–148 145 Table 1 Rock varnish development on blocks bigger than 10 cm randomly selected in deposit surfaces Landslide events N Rock varnish development o10 PA-1 PA-2 a b 500 300 400 10–50 50–90 490 x DS x DS x DS x DS 1.60 3.00 6.70 1.1 1.0 2.5 5.4 27.0 31.0 2.3 2.0 3.36 30.4 55.6 44.5 2.0 5.5 3.1 62.60 14.33 17.75 4.50 6.02 3.40 avalanches are absent in similar mountain fronts without active neotectonics. The TD and PA-1 events originate in mountain fronts affected by regional faults. These faults are associated with the Carrera fault system which has been active at least until Early Pleistocene (Kozlowski et al., 1993). Moreover, evidence of Quaternary activity of these faults has also been observed by Cortés et al. (1999). However, the relationship between rock avalanches and Quaternary fault activity is uncertain. Structural controls may also favor slope instability because the lithologies are affected by intense jointing. Highly fractured materials are liable to rapid and intense weathering because weakness zones enhance weathering and water movement, and thus favor potential planes of failure. Paleo-climatic conditions probably favored the occurrence of these events, as the TD rock avalanche occurred before formation of the Uspallata Glaciation outwash terrace. Periods of exceptionally warm temperature and severe rainfall force hillslope instability (Espizúa and Bengochea, 1991; Gonzalez Diez et al., 1996; Poschinger and Haas, 1997; Trauth and Strecker, 1999; Corsini et al., 2000, 2001; Trauth et al., 2000; Hermanns et al. 2000; Borgatti et al., 2001). The Uspallata glaciation is the oldest Pleistocene glaciation identified along the Rio Mendoza valley. This glaciation was assigned to at least Early Middle Pleistocene age because it is older than a tephra layer dated by fission track at 360736 ka (Espizúa, 1993) and older than a tephra layer intercalated in alluvial fans surrounding Uspallata terminal moraine in Uspallata valley dated 170750 ka (Espizúa and Bigazzi, 1998). Espizúa (1993) tentatively correlated this stage with the El Soldado glaciation, previously identified in the Aconcagua valley of Chile by Caviedes and Paskoff (1975). Thus, Espizúa and Bigazzi (1998) proposed that it could be correlated with the European prepenultimate glaciation, as the previous Punta de Vacas glaciation was correlated with penultimate glaciation and MIS 6. Nevertheless, several Pleistocene stadial periods have been identified in South America. Those studied in the Strait of Magellan (Tierra del Fuego) are estimated between 360 ka and 1.1 Myr old (Meglioli, 1992; Rabassa et al., 2000). Coronato et al. (2004a) identified a minimum of six regional glacial advances in Patagonia, from Late Pliocene–Early Pleistocene times to the Late Pleistocene and Late-glacial. In North Patagonia (411–431 South Latitude), two glaciations from Middle Pleistocene and the Great Patagonian Glaciation of Early Pleistocene in age have been identified. In Southern Patagonia (441300 –521S) different drifts that correspond to three glaciations of Middle Pleistocene age (Post-Great Patagonian Glaciation), the Great Patagonian Glaciation, and a Late Pliocene–Late Miocene glaciation have been identified (Coronato et al., 2004b). Kaplan et al. (2005) determined that different glaciations by cosmogenic measures in Lago Buenos Aires at 461 South Latitude correlated with MIS 2, 6, and 10 or 12. Glacial to interglacial changes and glacial maxima are global in Earth history, thus the glacial stages in the mid to high latitudes of South America coincide in timing with European and Northern American glaciations during at least the last 200,000 yr (Ackert et al., 2003; Douglass et al., 2005; Kaplan et al., 2004, 2005). However, local evidence and numerical dating is basically required to determine the precise age of the Uspallata Glaciation and interpret the existence of a prior interglacial stage. Paleo-climatic conditions could be determined by diatom analysis. Nevertheless, plant species identified in these outcroppings are cosmopolitan, and consequently climate conditions for the dammed-paleolake could not be determined. Future Quaternary studies in the region and numerical dating of involved deposits could enhance climatic influence evaluation. In summary, relation between the occurrence of PA-1 and TD rock avalanches and regional neotectonic activity is very probable. However, the link with Quaternary fault activity is more doubtful because large earthquakes can be effective at great distances (Voight and Pariseau, 1978; Keefer, 1984). Magnitude of the historical earthquake should have been higher than 6 according to the total volume of displaced material (Keefer, 1984; Keefer and Jibson, 1993). This hypothesis, based on neotectonic relationships, will extend seismic shakings in the region to the Middle Pleistocene time, and may also explain the occurrence of the younger PA-2. However, a climatic influence should not be underestimated. These findings match Hermanns and Strecker’s (1999) observations in other areas of the Central ARTICLE IN PRESS 146 S.M. Moreiras / Quaternary International 148 (2006) 138–148 Andes. These authors found that the trigger mechanism for the majority of 55 rock avalanches with volumes larger than 106 m3 and formed by the collapse of entire mountain fronts was seismic, although the age of some major slides are about 30 ka, which may correspond to a more humid interval in southern South America. Whether or not rock avalanches can be linked to Quaternary activity of the Placetas Amarillas and Piedras Blancas faults, they were active until Middle Pleistocene time. 14. Conclusion This research gives an approximate chronology of the Placetas Amarillas-1 (PA-1) and Tigre Dormido (TD) rock avalanches enhancing knowledge about these extraordinary events. Furthermore, a younger event is identified by geomorphology and relative age techniques. The PA-1 rock avalanche is at least of Middle Pleistocene age, as its deposit is overlain by an ash level dated at 350780 ka. As a similar age was proposed for the Tigre Dormido rock avalanche; temporal correlation of both rock avalanches is suggested. Thus, a common seismic triggering factor related to regional neotectonics is proposed in accordance with regional seismic activity. Although the occurrence of the PA-1 and TD rock avalanches is likely related to regional neotectonic activity, the climatic role should not be underestimated even lacking to support the existence of a warm period prior Uspallata glaciation. Commonly, analysis of climatic role is not easy in seismic regions, but it must be kept in mind that slope failures are generally influenced by a combination of factors such as lithological, structural and climatic conditions that predispose steep mountain fronts to failure (Schmidt and Dikau, 2004). Future efforts are geared towards numerical dating of rock avalanches and determining uncertainties about climatic influence. 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